2016
DOI: 10.1103/physrevd.94.054016
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Dipole factorization for DIS at NLO: Loop correction to theγT,L*qq¯light-front wave functions

Abstract: The one-loop QCD corrections to the light-front wave-function for the quark-antiquark Fock state inside a transverse or longitudinal off-shell photon are explicitly calculated, both in full momentum space and in mixed space (a.k.a. dipole space). These results provide one of the main contributions to virtual NLO corrections to many DIS observables (inclusive or not) in the dipole factorization formalism at low Bjorken x.In a follow-up article, these one-loop corrections are combined with earlier results on the… Show more

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Cited by 100 publications
(172 citation statements)
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References 84 publications
(215 reference statements)
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“…Derived via systematic approximations within perturbative QCD, the Colour Glass Condensate (CGC) effective theory [1][2][3][4][5] is a powerful framework for computing high-energy processes in the presence of nonlinear effects associated with high parton densities. There are intense ongoing efforts towards extending this effective theory to next-to-leading order (NLO) accuracy, as required by realistic applications to phenomenology [6][7][8][9][10][11][12][13][14][15][16][17][18][19]. These efforts refer both to the Balitsky-JIMWLK equations [20][21][22][23][24][25][26], which govern the high-energy evolution of the scattering amplitudes, and to the impact factors, which represent cross-sections at relatively low energy.…”
Section: Introductionmentioning
confidence: 99%
“…Derived via systematic approximations within perturbative QCD, the Colour Glass Condensate (CGC) effective theory [1][2][3][4][5] is a powerful framework for computing high-energy processes in the presence of nonlinear effects associated with high parton densities. There are intense ongoing efforts towards extending this effective theory to next-to-leading order (NLO) accuracy, as required by realistic applications to phenomenology [6][7][8][9][10][11][12][13][14][15][16][17][18][19]. These efforts refer both to the Balitsky-JIMWLK equations [20][21][22][23][24][25][26], which govern the high-energy evolution of the scattering amplitudes, and to the impact factors, which represent cross-sections at relatively low energy.…”
Section: Introductionmentioning
confidence: 99%
“…That calculation too was based on a factorization scheme nonlocal in rapidity (similar to the one that we employed in this paper) together with the NLO impact factor for the virtual photon from Refs. [32,33].…”
Section: The C F Termsmentioning
confidence: 99%
“…[31], a similar problem appears in the context of deep inelastic scattering (DIS), when using the "dipole factorization" (a version of k T factorization appropriate for DIS at high energy) together with the NLO impact factor from Refs. [32,33].…”
Section: Introductionmentioning
confidence: 99%
“…The numerical computation of the finite pieces con-stitutingX NLO;jet µν;finite , along with NLO BK/JIMWLK evolution, provide the necessary ingredients to compute photon+dijet production (and associated measurement channels) in e+A DIS to O(α 3 S ln(1/x)) accuracy. Prior NLO studies on DIS at small x focused on the crosssection for fully inclusive DIS [51][52][53][54][55][56][57][58][59], a noteworthy exception being the NLO studies of diffractive dijet and exclusive vector meson production by Boussarie et al [60][61][62]. In this regard, our work goes a step beyond by considering more differential final states.…”
mentioning
confidence: 95%